HSC 142

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0.30 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 18.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 142 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by very high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as genetic pair P127, along with HSC_152.

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 271.402 -18.938 0.558 1.42 0.618 -113.119
Hunt & Reffert 2024 271.405 -18.945 0.567 1.439 0.624 -113.137
Cavallo et al. 2024 271.44 -18.921 0.565 – – –
Hunt & Reffert 2023 271.405 -18.945 0.567 1.439 0.624 -113.137

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 1.895 5.17 2.46 94 0.850 467 – –
Hunt & Reffert 2024 – – – – – 467(1) – –
Cavallo et al. 2024 2.15 4.86 – 36 0.850 – – –
Hunt & Reffert 2023 1.64 5.48 2.46 152 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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